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Proceedings Paper • Open Access

Optical bench development for LISA
Author(s): L. d'Arcio; J. Bogenstahl; M. Dehne; C. Diekmann; E. D. Fitzsimons; R. Fleddermann; E. Granova; G. Heinzel; H. Hogenhuis; C. J. Killow; M. Perreur-Lloyd; J. Pijnenburg; D. I. Robertson; A. Shoda; A. Sohmer; A. Taylor; M. Tröbs; G. Wanner; H. Ward; D. Weise

Paper Abstract

For observation of gravitational waves at frequencies between 30 μHz and 1 Hz, the LISA mission will be implemented in a triangular constellation of three identical spacecraft, which are mutually linked by laser interferometry in an active transponder scheme over a 5 million kilometer arm length. On the end point of each laser link, remote and local beam metrology with respect to inertial proof masses inside the spacecraft is realized by the LISA Optical Bench. It implements further- more various ancillary functions such as point-ahead correction, acquisition sensing, transmit beam conditioning, and laser redundancy switching.

A comprehensive design of the Optical Bench has been developed, which includes all of the above mentioned functions and at the same time ensures manufacturability on the basis of hydroxide catalysis bonding, an ultrastable integration technology already perfected in the context of LISA's technology demonstrator mission LISA Pathfinder. Essential elements of this design have been validated by dedicated pre-investigations. These include the demonstration of polarizing heterodyne interferometry at the required Picometer and Nanoradian performance levels, the investigation of potential non-reciprocal noise sources in the so-called backlink fiber, as well as the development of a laser redundancy switch breadboard.

Paper Details

Date Published: 20 November 2017
PDF: 7 pages
Proc. SPIE 10565, International Conference on Space Optics — ICSO 2010, 105652X (20 November 2017); doi: 10.1117/12.2309141
Show Author Affiliations
L. d'Arcio, ESA, ESTEC (Netherlands)
J. Bogenstahl, Albert Einstein Institute (Germany)
M. Dehne, Albert Einstein Institute (Germany)
C. Diekmann, Albert Einstein Institute (Germany)
E. D. Fitzsimons, Univ. of Glasgow (United Kingdom)
R. Fleddermann, Albert Einstein Institute (Germany)
E. Granova, Albert Einstein Institute (Germany)
G. Heinzel, Albert Einstein Institute (Germany)
H. Hogenhuis, TNO Science and Industry (Netherlands)
C. J. Killow, Univ. of Glasgow (United Kingdom)
M. Perreur-Lloyd, Univ. of Glasgow (United Kingdom)
J. Pijnenburg, TNO Science and Industry (Netherlands)
D. I. Robertson, Univ. of Glasgow (United Kingdom)
A. Shoda, Albert Einstein Institute (Germany)
A. Sohmer, EADS Astrium GmbH - Satellites (Germany)
A. Taylor, Univ. of Glasgow (United Kingdom)
M. Tröbs, Albert Einstein Institute (Germany)
G. Wanner, Albert Einstein Institute (Germany)
H. Ward, Univ. of Glasgow (United Kingdom)
D. Weise, EADS Astrium GmbH - Satellites (Germany)


Published in SPIE Proceedings Vol. 10565:
International Conference on Space Optics — ICSO 2010
Errico Armandillo; Bruno Cugny; Nikos Karafolas, Editor(s)

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